A multiple spacecraft detection of the 2 April 2022 M-class flare and filament eruption during the first close Solar Orbiter perihelion (2023)

First Author: Janvier M
Attributed to:  How do weak shocks accelerate high energy particles? funded by STFC

Abstract

No abstract provided

Bibliographic Information

Digital Object Identifier: http://dx.doi.org/10.1051/0004-6361/202346321

Publication URI: http://dx.doi.org/10.1051/0004-6361/202346321

Type: Journal Article/Review

Parent Publication: Astronomy & Astrophysics